Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • Refereed
    Accretion processes in the galaxy cluster Hydra A/Abell 780
    Context. Clusters of galaxies evolve and accrete mass, mostly from small galaxy systems. Aims: Our aim is to study the velocity field of the galaxy cluster Abell 780, which is known for the powerful radio source Hydra A at its center and where a spectacular X-ray tail associated with the galaxy LEDA 87445 has been discovered. Methods: Our analysis
    Girardi, M. et al.

    Advertised on:

    2
    2022
    Bibcode
    2022A&A...658A.159G
    Citations
    2
  • Refereed
    A novel black hole mass scaling relation based on coronal gas, and its dependence with the accretion disc
    Using bona-fide black hole (BH) mass estimates from reverberation mapping and the line ratio [Si VI] 1.963$\rm{\mu m}$/Brγ broad as tracer of the AGN ionizing continuum, a novel BH-mass scaling relation of the form log(M BH) = (6.40 ± 0.17) - (1.99 ± 0.37) × log ([Si VI]/Brγ broad), dispersion 0.47 dex, over the BH mass interval, 10 6-10 8 M ⊙ is
    Prieto, Almudena et al.

    Advertised on:

    2
    2022
    Bibcode
    2022MNRAS.510.1010P
    Citations
    20
  • Refereed
    A multi-planetary system orbiting the early-M dwarf TOI-1238
    Context. The number of super-Earth and Earth-mass planet discoveries has increased significantly in the last two decades thanks to the Doppler radial velocity and planetary transit observing techniques. Either technique can detect planet candidates on its own, but the power of a combined photometric and spectroscopic analysis is unique for an
    González-Álvarez, E. et al.

    Advertised on:

    2
    2022
    Bibcode
    2022A&A...658A.138G
    Citations
    9
  • Refereed
    A candidate short-period sub-Earth orbiting Proxima Centauri
    Context. Proxima Centauri is the closest star to the Sun. This small, low-mass, mid M dwarf is known to host an Earth-mass exoplanet with an orbital period of 11.2 days within the habitable zone, as well as a long-period planet candidate with an orbital period of close to 5 yr. Aims: We report on the analysis of a large set of observations taken
    Faria, J. P. et al.

    Advertised on:

    2
    2022
    Bibcode
    2022A&A...658A.115F
    Citations
    78
  • Thesis
    A 3D VIEW OF AGN TRIGGERING
    Active galaxies are these showing strong emission coming from their nuclei. In the case of normal galaxies the nuclear emission has a stellar origin, but in active galactic nuclei (AGN) the emission is produced by accretion of matter into a super-massive black hole (SMBH). Although only a small percentage of galaxies in the nearby Universe
    Ignacio del Moral Castro

    Advertised on:

    2
    2022
    Bibcode
    THESIS
  • Thesis
    A 3D VIEW OF AGN TRIGGERING
    Active galaxies are these showing strong emission coming from their nuclei. In the case of normal galaxies the nuclear emission has a stellar origin, but in active galactic nuclei (AGN) the emission is produced by accretion of matter into a super-massive black hole (SMBH). Although only a small percentage of galaxies in the nearby Universe
    Ignacio del Moral Castro

    Advertised on:

    2
    2022
    Bibcode
    https://www.educacion.gob.es/teseo/mostrarSeleccion.do